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What stage is next when the sun finishes the main sequence stage?
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What occurs that causes a main sequence star to lose its equilibrium and move on to the next stage in its evolution?
This happens when a main sequence star uses up all of its fuel and swells. Next stage: Red Giant.
What is the present stage in the life of the sun?
The Main Sequence stage.
What happens to main sequence stars when energy from fusion is no longer available?
The star will move on to its next stage of evolution, along the Red Giant branch.
What stage is our sun in right now?
Our sun is a main sequence (dwarf) star. It's expected to remain so for the next 5 billion years or so. After that it will expand briefly into a red giant, then collapse into a white dwarf.
What is the suns next stage after 5 billion years?
Theoretically, in 5 billion years, the Sun will still be in the main sequence. 5.4 billion years (estimated) marks the end of main sequence, where it will be in the intermediary point between a main-sequence star and a post-main-sequence red giant, where it will slowly reach over 200 times it's current mass over the course of about a billion more years, at which point it would be classified as an official red giant and be fully burning helium-4 as a main source of fuel as well as burning a hydrogen shell it built up during the main-sequence. After that point it will eject most of its mass into a planetary nebula and slowly cool as a stellar remnant over the course of a few quadrillion years until it reaches 3K.
What occurs that causes a main sequence star to lose its equilibrium and move on to the next stage in its evolution?
This happens when a main sequence star uses up all of its fuel and swells. Next stage: Red Giant.
What is the present stage in the life of the sun?
The Main Sequence stage.
What is the next stage in the life of a lower-mass main-sequence star?
white dwarf. unless you count black dwarf of which none have been observed, only theorized.
What happens to main sequence stars when energy from fusion is no longer available?
The star will move on to its next stage of evolution, along the Red Giant branch.
What stage is our sun in right now?
Our sun is a main sequence (dwarf) star. It's expected to remain so for the next 5 billion years or so. After that it will expand briefly into a red giant, then collapse into a white dwarf.
What ful do stars on the main sequence burn?
it is fusion of hydrogen into helium. (like our sun) if it is a red giant (the next stage of our suns life) it is burning helium into denser things.
How does this sound for a main idea next you will go get groceries?
The word "next" tells the reader that this is not the main idea, because it is next in the sequence of the paragraph. There is a sentence before it that would be the main idea.
When the Sun moves off the main sequence it will next become a?
It will become a red giant.
What will a high mass protostar turn into?
A protostar is the first building block of the main star. As it has not yet accumulated enough mass to join the main sequence, it will be smaller than the main star. The next stage will be a T Tauri star.
What is the next letter in the sequence AAAAA?
The next letter in the sequence AAAAA is 'E'. It is a vowel sequence.
What is the next number in the sequence 124711.....?
What is the the next number in the sequence 1,2,4,7,11,.....
What is the suns next stage after 5 billion years?
Theoretically, in 5 billion years, the Sun will still be in the main sequence. 5.4 billion years (estimated) marks the end of main sequence, where it will be in the intermediary point between a main-sequence star and a post-main-sequence red giant, where it will slowly reach over 200 times it's current mass over the course of about a billion more years, at which point it would be classified as an official red giant and be fully burning helium-4 as a main source of fuel as well as burning a hydrogen shell it built up during the main-sequence. After that point it will eject most of its mass into a planetary nebula and slowly cool as a stellar remnant over the course of a few quadrillion years until it reaches 3K.
